The off-energy electron background disturbs the VSAT data in many ways, as will be discussed in section 4.1 the coincidence of two off-energy electrons can trigger a Bhabha event. This ``false Bhabha'' rate normally stays below 30% of the number of Bhabha triggers, but can at times go above 50% (Fig. 3.6). Most of the false Bhabhas can be removed with narrow cuts due to the well confined properties of a true Bhabha event. The remaining background can be quantized by a linear combination of four different measurements [16]:
Here Ecut is the number of events cut away by the Bhabha
energy cut, S and SE the number of downscaled off-energy electron
triggers with and without the energy cut. The duration of the
measured data is given by T and
Bsoft - Bhard is
the difference between the normal Bhabha sample and one with
especially hard background cuts. Finally the FBscal is the
online delayed Bhabha scaler (taken as the coincidence of two
opposite hits separated by four bunch crossings), which only is usable
in cases of bad statistics.
A
-event is triggered by cuts on the hadronic system
in the DELPHI detector (section 5.1). If an off-energy
electron coincides with the hadronic trigger, it can result in any
of the following VSAT
-event:
The most troublesome background for this analysis is the second
, as the confinement of the off-energy background is mixed up
with the spread of true
-events. The other two
background triggers could in principle be completely removed by
strong cuts, without too much loss of the signal. This is not
possible for second type and the size of the background has to be
estimated in order to make an efficiency calculation.